One-dimensional hydrodynamical simulations of gravitational clustering in an expanding background.

Details One-dimensional hydrodynamical simulations of gravitational clustering in an expanding background. One-dimensional hydrodynamical simulations of gravitational clustering in an expanding background.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apl%26c..33...71p&link_type=abstract

Astrophysical Letters and Communications, Vol. 33, Nos. 1 - 5, p. 71 - 77

Astronomy and Astrophysics

Astrophysics

Galaxy Clustering: N-Body Simulations, Dark Matter: Universe

Scientific paper

The authors present the results of a series of one-dimensional N-body and hydrodynamical simulations which have been used for testing the different clustering properties of baryonic and dark matter in an expanding background. Initial Gaussian random density perturbations with a power-law spectrum are assumed. They analyse the distribution of density fluctuations and thermodynamical quantities for different spectral indices and discuss the statistical properties of clustering in the corresponding simulations.

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